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Table 1.

Non-magnetic CVs found in the RBS.

RBS# Name (pc) fX (erg cm−2 s−1) p (mas) Δp (mas) log LX (s−1) D (pc) Dmax (pc) Vgen (pc3)
2 EF Tuc 500: 32.0 3.38E–12 0.720 0.023 32.9 1335 1462 2.09E+08
22 WW Cet 100 31.0 9.16E–12 4.588 0.047 31.7 216 389 3.28E+07
280 TT ARI 135 31.1 5.96E–12 3.884 0.070 31.7 256 372 4.20E+07
288 WX HYI 265 31.6 6.26E–12 4.273 0.029 31.6 232 346 3.21E+07
372 IQ Eri 130 30.8 3.76E–12 5.186 0.167 31.2 192 222 1.11E+07
490 33 29.6 3.36E–12 3.098 0.126 31.6 320 349 3.51E+07
512 VW Hyi 65 30.9 1.59E–11 18.531 0.022 30.7 54 128 3.26E+06
664 TW Pic 3.13E–12 2.284 0.022 31.8 432 455 7.99E+07
694 SU UMa 280 32.1 1.41E–11 4.535 0.029 31.9 219 490 9.25E+07
710 SW UMa 140 30.9 3.81E–12 6.148 0.080 31.1 162 188 9.09E+06
(713 EI UMa)
728 BZ UMa 110 30.9 6.12E–12 6.557 0.064 31.2 152 224 1.39E+07
1008 T Leo 100 31.1 9.88E–12 7.814 0.069 31.3 128 240 1.33E+07
1411 RHS40 460 32.0 3.47E–12 2.919 0.671 31.7 367 407 3.72E+07
1900 TY PsA 300: 31.7 4.68E–12 5.431 0.065 31.3 183 236 1.26E+07
1955 V405 Peg 30 29.5 3.05E–12 5.784 0.062 31.0 172 179 8.06E+06
1969 CC Scl 165 31.1 4.23E–12 4.904 0.148 31.3 203 249 1.37E+07

Notes. #713 is no longer considered non-magnetic, whereas #664 was previously classified as an IP. The luminosity is given in the ROSAT spectral band 0.1–2.4 keV. Distances and luminosities from Schwope et al. (2002) are listed in columns with tildes, all other values are from this work. Vgen was computed for a scale height of 200 pc.

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